K stars more likely to host habitable exoplanets

By Brooks Hays
An artists concept of a planet orbiting in the habitable zone of a K star. Image by Tim Pyle/JPL-Caltech/NASA Ames
An artists concept of a planet orbiting in the habitable zone of a K star. Image by Tim Pyle/JPL-Caltech/NASA Ames

March 8 (UPI) -- Scientists have dubbed K stars "Goldilocks stars." According to a new study, K stars are more likely to host habitat exoplanets than other types of stars.

If life is to be found outside planet Earth, the new research suggests K stars are where astronomers should look. K stars are orangish stars that register a bit cooler than the sun.


There are billions of stars in the universe. Astronomers looking for signs of alien life can barely scratch the surface of the universe's stellar population. The new research promises to narrow astronomers' search parameters.

As detailed in the Astrophysical Journal Letters, K stars have several advantages. They live a long time, providing surrounding planets plenty of time for the development of life. More importantly, K stars feature less electromagnetic turbulence.

RELATED Stellar third wheel can boost the habitable zone in binary star systems

The larger, more frequent solar flares produced by M stars can strip away the atmosphere of inner planets, quashing the chance for the development of life.

"I like to think that K stars are in a 'sweet spot' between Sun-analog stars and M stars," Giada Arney, a planetary scientist at NASA's Goddard Space Flight Center, said in a news release.


Scientists developed models to predict what biosignatures might look like in the atmosphere of an exoplanet orbiting a K star. Because oxygen and methane typically destroy each other, their simultaneous atmospheric presence suggests some type of process -- possibly a biological one -- is continually producing the two gases.

RELATED Custom frequency comb to improve precision of planet-hunting telescope

Oxygen and methane can be hard to spot from thousands of light-years away, but the models created by Arney and her colleagues showed oxygen-methane biosignatures would be more evidence the atmosphere of exoplanets in K star systems.

"When you put the planet around a K star, the oxygen does not destroy the methane as rapidly, so more of it can build up in the atmosphere," said Arney. "This is because the K star's ultraviolet light does not generate highly reactive oxygen gases that destroy methane as readily as a Sun-like star."

Because K stars are dimmer, the exoplanets orbiting them should be easier to spot. In their new paper detailing habitability in K star planetary systems -- published this week in the Astrophysical Journal -- authors identified several nearby K stars to be explored during future astronomical surveys.

RELATED First-ever exoplanet collision observed in Kepler 107 system

"I find that certain nearby K stars like 61 Cyg A/B, Epsilon Indi, Groombridge 1618, and HD 156026 may be particularly good targets for future biosignature searches," said Arney.


Latest Headlines